{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2013:EENGGNH6SFNSRQYLNCJ52LZBVO","short_pith_number":"pith:EENGGNH6","canonical_record":{"source":{"id":"1302.0005","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-01-31T21:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"0a204bf40b66e274e4b7d69b6ba40d115d79129b3daec2d7a4ab536b2ba47ebf","abstract_canon_sha256":"3d642a49ef84d52f81b70b69f4803326202079f0214b586fda06f6449c110dfe"},"schema_version":"1.0"},"canonical_sha256":"211a6334fe915b28c30b6893dd2f21ab9b3552d223a6129a002374e1c7abb6e6","source":{"kind":"arxiv","id":"1302.0005","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1302.0005","created_at":"2026-05-18T01:51:56Z"},{"alias_kind":"arxiv_version","alias_value":"1302.0005v2","created_at":"2026-05-18T01:51:56Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1302.0005","created_at":"2026-05-18T01:51:56Z"},{"alias_kind":"pith_short_12","alias_value":"EENGGNH6SFNS","created_at":"2026-05-18T12:27:43Z"},{"alias_kind":"pith_short_16","alias_value":"EENGGNH6SFNSRQYL","created_at":"2026-05-18T12:27:43Z"},{"alias_kind":"pith_short_8","alias_value":"EENGGNH6","created_at":"2026-05-18T12:27:43Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2013:EENGGNH6SFNSRQYLNCJ52LZBVO","target":"record","payload":{"canonical_record":{"source":{"id":"1302.0005","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-01-31T21:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"0a204bf40b66e274e4b7d69b6ba40d115d79129b3daec2d7a4ab536b2ba47ebf","abstract_canon_sha256":"3d642a49ef84d52f81b70b69f4803326202079f0214b586fda06f6449c110dfe"},"schema_version":"1.0"},"canonical_sha256":"211a6334fe915b28c30b6893dd2f21ab9b3552d223a6129a002374e1c7abb6e6","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:51:56.484799Z","signature_b64":"jfPaPYCSD6aYApmAJCPuiEXnapH0Mfxw0v8l5wfj7t19EqDk6Qz38J24I2ppAxh4aDdhYELKPbl9v4EbT/GeBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"211a6334fe915b28c30b6893dd2f21ab9b3552d223a6129a002374e1c7abb6e6","last_reissued_at":"2026-05-18T01:51:56.484171Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:51:56.484171Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1302.0005","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:51:56Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ugksbMvfa1TKAK5IMNzhiIChNr5CS0G/8HtENXETcy91GEU6BaLRKDoDwLlWBrUYywi0/2/ICue2h6uSOQ2RDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-07-02T17:04:56.515837Z"},"content_sha256":"aa55301a631a683e0106c20c8469e75ba43f1c2d9daf00f0a512f7a65531fb7a","schema_version":"1.0","event_id":"sha256:aa55301a631a683e0106c20c8469e75ba43f1c2d9daf00f0a512f7a65531fb7a"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2013:EENGGNH6SFNSRQYLNCJ52LZBVO","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"The Galaxy-Halo/Subhalo connection: Mass relations and implications for some satellite occupational distributions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Rodriguez-Puebla, N. Drory (IA-UNAM), V. Avila-Reese","submitted_at":"2013-01-31T21:00:01Z","abstract_excerpt":"We infer the local stellar-to-halo/subhalo mass relations (MRs) for central and satellite galaxies separately. We constraint this relations by using several combinations of observational data, consisting of the total galaxy stellar mass function, its decomposition into centrals and satellites, and the projected two-point correlation functions measured in different stellar mass bins. The differences among the resulting MRs are within the model-fit uncertainties (which are very small, smaller than the intrinsic scatter between galaxy and halo mass), no matter what combination of data are used. W"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1302.0005","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:51:56Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"WXcPwEH5TaoatJQydMJ+48/FjMJZJ9WR8Wzer3YwO7yTIOatUAqvH6hu6kNQ6so3fvcGSWLxf68JtKQpM3CPBg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-07-02T17:04:56.516181Z"},"content_sha256":"fa2b6774438b50a29fbbb39707be8619303c818697d58827ceb7dc78c075fc83","schema_version":"1.0","event_id":"sha256:fa2b6774438b50a29fbbb39707be8619303c818697d58827ceb7dc78c075fc83"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/EENGGNH6SFNSRQYLNCJ52LZBVO/bundle.json","state_url":"https://pith.science/pith/EENGGNH6SFNSRQYLNCJ52LZBVO/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/EENGGNH6SFNSRQYLNCJ52LZBVO/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-07-02T17:04:56Z","links":{"resolver":"https://pith.science/pith/EENGGNH6SFNSRQYLNCJ52LZBVO","bundle":"https://pith.science/pith/EENGGNH6SFNSRQYLNCJ52LZBVO/bundle.json","state":"https://pith.science/pith/EENGGNH6SFNSRQYLNCJ52LZBVO/state.json","well_known_bundle":"https://pith.science/.well-known/pith/EENGGNH6SFNSRQYLNCJ52LZBVO/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2013:EENGGNH6SFNSRQYLNCJ52LZBVO","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"3d642a49ef84d52f81b70b69f4803326202079f0214b586fda06f6449c110dfe","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-01-31T21:00:01Z","title_canon_sha256":"0a204bf40b66e274e4b7d69b6ba40d115d79129b3daec2d7a4ab536b2ba47ebf"},"schema_version":"1.0","source":{"id":"1302.0005","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1302.0005","created_at":"2026-05-18T01:51:56Z"},{"alias_kind":"arxiv_version","alias_value":"1302.0005v2","created_at":"2026-05-18T01:51:56Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1302.0005","created_at":"2026-05-18T01:51:56Z"},{"alias_kind":"pith_short_12","alias_value":"EENGGNH6SFNS","created_at":"2026-05-18T12:27:43Z"},{"alias_kind":"pith_short_16","alias_value":"EENGGNH6SFNSRQYL","created_at":"2026-05-18T12:27:43Z"},{"alias_kind":"pith_short_8","alias_value":"EENGGNH6","created_at":"2026-05-18T12:27:43Z"}],"graph_snapshots":[{"event_id":"sha256:fa2b6774438b50a29fbbb39707be8619303c818697d58827ceb7dc78c075fc83","target":"graph","created_at":"2026-05-18T01:51:56Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"We infer the local stellar-to-halo/subhalo mass relations (MRs) for central and satellite galaxies separately. We constraint this relations by using several combinations of observational data, consisting of the total galaxy stellar mass function, its decomposition into centrals and satellites, and the projected two-point correlation functions measured in different stellar mass bins. The differences among the resulting MRs are within the model-fit uncertainties (which are very small, smaller than the intrinsic scatter between galaxy and halo mass), no matter what combination of data are used. W","authors_text":"A. Rodriguez-Puebla, N. Drory (IA-UNAM), V. Avila-Reese","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-01-31T21:00:01Z","title":"The Galaxy-Halo/Subhalo connection: Mass relations and implications for some satellite occupational distributions"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1302.0005","kind":"arxiv","version":2},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:aa55301a631a683e0106c20c8469e75ba43f1c2d9daf00f0a512f7a65531fb7a","target":"record","created_at":"2026-05-18T01:51:56Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"3d642a49ef84d52f81b70b69f4803326202079f0214b586fda06f6449c110dfe","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-01-31T21:00:01Z","title_canon_sha256":"0a204bf40b66e274e4b7d69b6ba40d115d79129b3daec2d7a4ab536b2ba47ebf"},"schema_version":"1.0","source":{"id":"1302.0005","kind":"arxiv","version":2}},"canonical_sha256":"211a6334fe915b28c30b6893dd2f21ab9b3552d223a6129a002374e1c7abb6e6","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"211a6334fe915b28c30b6893dd2f21ab9b3552d223a6129a002374e1c7abb6e6","first_computed_at":"2026-05-18T01:51:56.484171Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:51:56.484171Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"jfPaPYCSD6aYApmAJCPuiEXnapH0Mfxw0v8l5wfj7t19EqDk6Qz38J24I2ppAxh4aDdhYELKPbl9v4EbT/GeBw==","signature_status":"signed_v1","signed_at":"2026-05-18T01:51:56.484799Z","signed_message":"canonical_sha256_bytes"},"source_id":"1302.0005","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:aa55301a631a683e0106c20c8469e75ba43f1c2d9daf00f0a512f7a65531fb7a","sha256:fa2b6774438b50a29fbbb39707be8619303c818697d58827ceb7dc78c075fc83"],"state_sha256":"14960d005714afab7e4c8086c792a97bf9d04a1165d6aa0da1cd42cd9628ebb5"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"tXOV1S/qLF5P+B5fB8F4UcAkEOWbIIcZ9R9eLjnvwfS3bxyS+GeFlH77C4lpfZia2roXnE5k6+Wo2PTyNyRqCg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-07-02T17:04:56.518148Z","bundle_sha256":"9c11e4262eb5fc358d0702734f0999bb18934601fa8136a788e3f93cf98a1275"}}